activity
20092021
most citedEffective Temperatures of Cataclysmic Variable White Dwarfs as a Probe of their Evolution

99 citations · 333 across the 14 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2021

Optical Variability Correlated with X-ray Spectral Transition in the Black-Hole Transient ASASSN-18ey = MAXI J1820+070

Keito Niijima, Mariko Kimura, Yasuyuki Wakamatsu +49

How a black hole accretes matter and how this process is regulated are fundamental but unsolved questions in astrophysics. In transient black-hole binaries, a lot of mass stored in…

astro-ph.EP202137 cited

Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b

Rebekah I. Dawson, Chelsea X. Huang, Rafael Brahm +53

TOI-216 hosts a pair of warm, large exoplanets discovered by the TESS Mission. These planets were found to be in or near the 2:1 resonance, and both of them exhibit transit timing…

astro-ph.SR2020

IM Normae: The Death Spiral of a Cataclysmic Variable?

Joseph Patterson, Jonathan Kemp, Berto Monard +18

We present a study of the orbital light curves of the recurrent nova IM Normae since its 2002 outburst. The broad "eclipses" recur with a 2.46 hour period, which increases on a tim…

astro-ph.SR2020

The Spin-Period History of Intermediate Polars

Joseph Patterson, Enrique de Miguel, Jonathan Kemp +25

We report the detailed history of spin-period changes in five intermediate polars (DQ Herculis, AO Piscium, FO Aquarii, V1223 Sagittarii, and BG Canis Minoris) during the 30-60 yea…

astro-ph.SR20193 cited

Infrared spectroscopy of the recent outburst in V1047 Cen (Nova Centauri 2005)

T. R. Geballe, D. P. K. Banerjee, A. Evans +14

Fourteen years after its eruption as a classical nova (CN), V1047 Cen (Nova Cen 2005) began an unusual re-brightening in 2019 April. The amplitude of the brightening suggests that…

astro-ph.EP201936 cited

TOI-216b and TOI-216c: Two warm, large exoplanets in or slightly wide of the 2:1 orbital resonance

Rebekah I. Dawson, Chelsea X. Huang, Jack J. Lissauer +32

Warm, large exoplanets with 10-100 day orbital periods pose a major challenge to our understanding of how planetary systems form and evolve. Although high eccentricity tidal migrat…